The galaxy presents a generally smooth morphology, appearing largely elliptical in shape. The light distribution is concentrated towards the center, exhibiting a bright, yellowish core. There is a noticeable color gradient, transitioning from the yellowish central region to a redder outer halo. Faint, diffuse extensions of light are observed at the edges of the galaxy, suggestive of a spheroidal structure. There is very little evidence of spiral arms or prominent dust lanes within the galaxy's structure. The galaxy appears relatively isolated, with no obvious signs of major mergers or significant tidal distortions. There may be some minor disturbances visible that could be the result of a minor merger. Overall, the galaxy's visual properties point to a relatively evolved system, likely dominated by an older stellar population.
