The galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. The light distribution is centrally concentrated, with a noticeable, but not extreme, decline in surface brightness towards the outer regions. The galaxy appears to be dominated by an older stellar population, indicated by its redder color, though some blue light is visible. There is a secondary concentration of light, which may indicate a galactic nucleus. No spiral arms, dust lanes, or other signs of recent star formation activity are readily apparent. The overall structure suggests a quiescent system, potentially an elliptical galaxy nearing the end of its evolutionary lifecycle. There are no signs of tidal disturbances or interaction with nearby galaxies.
