The galaxy presents as a somewhat diffuse, centrally concentrated object, exhibiting a near-elliptical morphology. The core region appears smooth and lacks any distinct, well-defined spiral arm structure. There appears to be evidence of faint, diffuse features extending outward, perhaps suggesting tidal disturbances or ongoing minor interactions. The central region has a yellowish hue, possibly indicative of an older stellar population, while the faint outer regions exhibit a bluer color profile suggesting areas of more recent star formation, or potential tidal debris. There are no obvious signs of a prominent dust lane or bar structure within the galaxy's disk.
