The galaxy presents as a system with a primarily smooth morphology. The central region exhibits a relatively high surface brightness, appearing as a concentrated bulge.  The outer regions gradually fade into the background sky, lacking distinct spiral arms or other prominent features indicative of a strong disk component. There may be hints of faint, diffuse extensions or tidal features, but the overall structure suggests a galaxy undergoing a phase of relatively quiescent evolution. The color profile appears relatively uniform across the galaxy, with a slight reddening towards the central bulge, consistent with an older stellar population in that region. No strong signs of active star formation are immediately apparent from the visual data alone, suggesting that the galaxy's star formation rate may be low. It is possible there may have been a merger in the past, but there does not seem to be any current merging events occurring.
