The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and rounded morphology. The light profile appears centrally concentrated, with a gradual decline in surface brightness moving outwards from the core. The galaxy’s color is generally yellowish-white, suggesting an older stellar population with a lower rate of ongoing star formation. There are no prominent spiral arms, bar structures, or significant dust lanes visible within the galaxy's structure. Faint extensions or tidal features are not apparent, indicating a lack of recent major merger activity. The galaxy appears relatively isolated, with no obvious signs of strong gravitational interaction with nearby companions.
