The galaxy presents an overall smooth, elliptical morphology. Its core appears relatively bright and concentrated, exhibiting a yellowish-orange hue, suggesting a population of older stars and a relatively low rate of ongoing star formation in this region. Moving outward from the core, the light gradually diffuses, with a subtle color gradient, transitioning to a slightly redder tone. There is a faint extension or possible tidal tail that stretches out from the main body. The feature shows hints of blue, which could indicate the presence of a younger stellar population or regions of recent star formation. The elongation of the galaxy suggests that it is likely not perfectly spherical but rather somewhat flattened or cigar shaped. There may be some minor disturbances in the disk, suggesting interactions with a smaller galaxy or object.
