The galaxy presents as a generally smooth, elliptical morphology. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue, which may indicate a population of older stars. A faint, diffuse disk is perceptible surrounding the bulge. This disk appears less structured and contains a lower surface brightness compared to the central region. There is no strong evidence of spiral arms or significant dust lanes. The color gradient suggests a decrease in star formation rate, with the central regions likely dominated by older stellar populations. The overall structure appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions, though there are subtle hints of minor disturbances. The ellipticity indicates it is not a perfect sphere. The size suggests a moderately sized galaxy.
