The galaxy presents as an elliptical or lenticular morphology. The light distribution is smooth and centrally concentrated, exhibiting a gradual falloff in surface brightness from the core to the outer regions. The isophotes appear largely regular. There are no prominent spiral arms, bar features, or significant dust lanes visible. The galaxy exhibits a moderate red color, suggesting an older stellar population with a relatively low rate of on-going star formation. Faint tidal features or distortions may be present at a subtle level, potentially indicating past or ongoing interactions with other galaxies.
