This galaxy presents as an elliptical or lenticular type, showing a smooth, concentrated light profile with minimal discernible internal structure. It is elongated, with a noticeable axis ratio indicating a deviation from perfect sphericity. The galaxy exhibits a yellowish-red color, suggesting an older stellar population with a lower rate of ongoing star formation. There are no apparent spiral arms, dust lanes, or prominent star-forming regions visible in this image. The galaxy appears relatively isolated with no obvious signs of tidal interactions or major disturbances.
