The galaxy presents as a centrally concentrated, elliptical or lenticular system, exhibiting a smooth, relatively featureless morphology. The luminosity profile appears to peak sharply at the core, suggesting a dense nucleus. The galaxy has a generally round shape with a very slight elongation. The light distribution indicates a dominant older stellar population, with a redder hue in the central regions, possibly suggesting a greater concentration of older, less massive stars and dust. There is little evidence of ongoing star formation. The galaxy appears isolated, showing no signs of tidal disturbances or interaction with neighboring galaxies, lending support to its classification as a non-merging system.
