The galaxy presents as a relatively smooth, elliptical morphology. Its overall shape is moderately elongated, exhibiting an aspect ratio suggestive of an E4-E5 classification on the Hubble sequence. There is a subtle color gradient across the galaxy, transitioning from a more yellow/orange hue in the core region to a slightly bluer tinge in the outer regions. This color variation could indicate a degree of ongoing star formation within the galaxy, although the dominant stellar population appears to be older, contributing to the yellow/orange color. There are no prominent spiral arms or distinct dust lanes visible. Faint hints of disturbed structure suggest possible minor interactions with nearby galaxies. The galaxy does not appear to be undergoing a major merger event.
