The galaxy appears as a luminous, centrally concentrated object. It exhibits a largely smooth morphology, with a generally elliptical shape. There is a hint of a disk structure. The light distribution suggests a bulge component, possibly a supermassive black hole, but the low resolution makes it difficult to determine. There is a color gradient across the galaxy, with the core appearing yellower and redder at the edges, suggesting a difference in stellar population distribution; the core possibly has older, redder stars. There is little evidence of active star formation regions, indicating that it may be a relatively quiescent galaxy. There is a possibility of minor disturbances to the structure from tidal interactions with other galaxies in the area, but more information is needed.
