The galaxy exhibits a primarily smooth morphology, with a somewhat elongated, cigar-shaped appearance. It presents a concentrated central bulge that graduates into a more diffuse halo. A slight disclike structure appears present upon observation of colors and faint structural characteristics. The color profile indicates a relatively even distribution of stellar populations, with a tendency towards slightly bluer hues. It is unlikely a galaxy undergoing major merger activity. There is a low probability of tidal interactions or the presence of prominent, extended tidal tails. Faint, but present, features may indicate minor gravitational disturbance.
