The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with brightness decreasing gradually towards the outer edges. The galaxy appears nearly circular in shape. There is minimal evidence of spiral arm structure or prominent dust lanes. There are no obvious signs of any ongoing major mergers or significant tidal disturbances affecting its structure. Color gradients across the galaxy are subtle, with the central region appearing slightly bluer than the outer regions. This might indicate a higher concentration of younger stars in the core, although the overall color suggests a generally older stellar population. There is a very slight chance it might have an extremely faint disc. The galaxy appears to be relatively isolated, showing no obvious interactions with any nearby companion galaxies.
