The galaxy presents as a concentrated elliptical morphology with a smooth light profile, suggesting an older stellar population. The galaxy exhibits a noticeable central bulge with a gradual decrease in luminosity outwards, which blends smoothly into the outer regions. Its shape is elongated. There are no obvious signs of spiral arms, active star formation, or significant dust lanes visible in this image. This supports the classification of the galaxy as an elliptical or lenticular type, dominated by evolved stars and low star formation activity. No signs of major disturbances or interactions with other galaxies are discernible.
