The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, brighter luminosity, suggesting a prominent galactic nucleus. There is a slight elongation in the shape, deviating somewhat from a perfectly circular form. The galaxy displays a color gradient, with the central core appearing more yellowish-white, and the outer regions trending towards a bluer hue. There are subtle indications of internal structures, potentially weak spiral arms or dust lanes, though these features are not sharply defined. No clear evidence of strong tidal interactions or major mergers are immediately apparent, though some minor disturbance may be possible. Star formation appears relatively low, although a range is possible given the data.
