The galaxy presents as a centrally concentrated, elliptical-like object with a relatively smooth light distribution. It appears approximately round, with a slight elongation that is difficult to discern at this resolution. The central region exhibits a bright, yellowish hue, possibly indicative of an older stellar population or significant dust obscuration. There appears to be very little, if any, evidence of spiral arm structure or prominent star-forming regions. A faint, diffuse halo surrounds the central bulge, fading into the background sky. There is some minor indication of gravitational interaction. It appears as a small, redder object very close to the subject.
