The galaxy presents as a mostly smooth, elliptical-like structure with a dominant central bulge. This central region exhibits a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. A faint disk-like component is visible, oriented nearly edge-on to our line of sight. This disk is subtle, with limited evidence of distinct spiral arm features. The overall color profile leans towards redder hues, implying a population of older stars and a relatively low rate of ongoing star formation. There may be minor disturbances or irregularities in its outer regions, though the primary structure appears relatively undisturbed. The galaxy does not appear to be undergoing a major merging event. It is slightly elongated, but the overall morphology is generally round.
