The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance. A bright, yellowish core is dominant, suggesting a significant population of older stars within the nuclear region. The galaxy exhibits a somewhat elliptical shape, with a moderate degree of roundness. There is a faint, diffuse outer halo extending from the central region. The overall color index suggests the presence of older stellar populations, and the lack of prominent spiral arms or dust lanes indicates the galaxy is likely an elliptical or lenticular type. There is no clear evidence of strong tidal interactions or recent major mergers, although there are slight disturbances, but there may be recent or ongoing minor mergers, or tidal effects, that have given rise to some subtle distortions. The colors present throughout the image suggest that it is a typical galaxy in its redshift, with no strong indication of unusually intense star formation, but there may be some star formation occurring. The lack of blue regions suggests there are no large clusters of young, hot stars.
