The galaxy presents as a relatively smooth, elliptical or lenticular structure. It has a concentrated central bulge, characterized by a bright, yellowish hue, indicative of an older stellar population. There appears to be a faint, diffuse halo extending outward from the central region. This outer region exhibits a redder color compared to the core. There is no evidence of prominent spiral arms or distinct dust lanes. Overall, the galaxy appears undisturbed, showing no signs of recent major mergers or tidal interactions.
