The galaxy exhibits a generally smooth morphology, with a diffuse, elliptical shape. Its core region presents a bright, concentrated luminosity, transitioning outwards to a more subdued halo. The color profile indicates a dominant population of older stars, suggested by the redder hues, with potentially a moderate amount of ongoing star formation activity evidenced by slightly bluer regions within the disk, which contributes to a mixed yellowish hue. Slight disturbances in the otherwise smooth profile indicates a possible recent minor interaction, but it is not currently undergoing a major merging event. The elongated shape suggests a moderate degree of inclination relative to our line of sight.
