The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The galaxy exhibits a yellowish hue, indicative of a population of older stars, which are dominant in elliptical galaxies. There is little evidence of spiral arms or significant dust lanes, further supporting an elliptical classification. The shape is tending towards round, but is slightly in between round and elongated. A faint extension or tidal tail is visible towards the left of the galaxy, suggesting a possible minor interaction or past merger event. There are no obvious signs of ongoing major disturbances or mergers in the primary body of the galaxy. The galaxy appears relatively isolated with no close companions visible in this image.
