The galaxy presents as a relatively compact, smooth structure with a slightly elliptical morphology. There appears to be a well-defined central bulge that is more luminous compared to the outer regions of the galactic disc, which suggests it is composed of older stars. The galaxy exhibits a yellow-white hue, indicative of a moderate amount of star formation activity. No prominent spiral arm structure is discernible. The overall appearance suggests a galaxy in transition. There are some minor disturbances to the galaxy's symmetrical shape, indicating there may have been a minor merger, or there are signs of tidal disruption.
