The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. The light distribution appears relatively uniform, with a subtle elongation suggesting a slight deviation from a perfect spherical shape. There is no readily discernible spiral arm structure or prominent dust lanes. The color is generally uniform across the galaxy, trending towards redder hues, with a peak wavelength in the orange-red region. This suggests a stellar population dominated by older, evolved stars, implying that the galaxy's star formation rate may be relatively low or quiescent. There is no clear evidence of tidal disturbances or ongoing mergers, though a possible faint extension can be seen to the left side of the central galaxy.