The galaxy presents as a flattened ellipsoid, strongly suggesting an elliptical morphology or a late stage spiral galaxy viewed edge-on. The central region exhibits a bright, concentrated luminosity profile, indicating a significant stellar population and possibly an active galactic nucleus or a substantial black hole at its core. Moving outwards from the center, the light gradually fades into a more diffuse halo. The light distribution is not perfectly smooth, showing some irregularities and possible signs of substructure, which may be indicative of past merger events or ongoing tidal interactions. The overall color appears to be reddish-yellow, characteristic of older stellar populations. There is no visible evidence of distinct spiral arms, dust lanes, or prominent star-forming regions. 
