The galaxy presents as a relatively small, elliptical structure, with a noticeable central bulge that appears significantly brighter than the surrounding regions. Its overall shape is elongated, displaying a cigar-like form, and appears to be relatively smooth in texture with no prominent spiral arms or distinct features. The color gradient suggests a bluer central region, possibly indicative of a younger stellar population or ongoing star formation concentrated near the core. The outer regions exhibit a redder hue, which could signify an older stellar population. No tidal tails or obvious signs of recent merger activity are apparent, suggesting it is a relatively undisturbed system.
