The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a primarily elliptical morphology, appearing largely rounded with a slight elongation. The color profile indicates a redder hue, particularly towards the core, suggesting an older stellar population. The galaxy appears to lack prominent spiral arm structures or significant dust lanes. A faint, diffuse halo seems to extend from the central bulge, gradually fading into the background. There is no obvious evidence of ongoing major merger activity, although subtle asymmetries might indicate minor past interactions. Star formation appears to be relatively low.
