The galaxy presents as a centrally concentrated object with a smooth light distribution, indicating a likely elliptical or lenticular morphology. The galaxy exhibits a slightly elongated shape and a relatively small angular size, consistent with its estimated distance. The light profile appears to be relatively uniform across the galaxy's body with a bright central point. There is no clear evidence of spiral arm structure, dust lanes, or significant star-forming regions. There may be a very slight disturbance or tidal feature present but it is difficult to discern, suggesting a potentially ongoing or past minor interaction. The overall color appears to be fairly uniform across the galaxy, with subtle variations in hue. The apparent magnitude suggests an intrinsically luminous object, potentially indicating a large stellar mass and a moderate amount of star formation activity, although it's likely dominated by an older stellar population given its morphology.
