The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge, indicating a relatively evolved system. The color profile suggests a dominant population of older stars, likely red giants and dwarfs, contributing to its yellowish-orange hue. There is little evidence of strong spiral arm structure or significant dust lanes. The galaxy appears somewhat rounded in shape, showing no significant elongation or distortion that would suggest a recent major merger event, although there seems to be minor disturbances present.
