The galaxy presents as a relatively compact object. There is a slight central concentration of light, suggesting a bulge, but it is not sharply defined. The overall color appears to be on the redder side, which may indicate an older stellar population. There seems to be some evidence of tidal disturbances or faint plumes extending from the main body, possibly suggesting interaction with another galaxy or past merger events. These features are subtle, however, and could also be artifacts. The light profile is somewhat irregular, displaying only the slightest hint of spiral arm structure or a disk. Overall, the galaxy's morphology points towards it being an elliptical or lenticular galaxy with potential signs of recent or ongoing tidal interaction.
