The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light profile indicates a single, dominant component, lacking prominent spiral arms or a distinct bar structure. The overall shape appears more elliptical than disk-like, though not perfectly spherical. The color is relatively uniform across the visible portion of the galaxy, displaying a yellow-orange hue. This coloration suggests a stellar population dominated by older, cooler stars, implying a relatively low rate of ongoing star formation. There is no obvious indication of dust lanes, tidal features, or recent merger activity. The galaxy exhibits a slight elongation, but it is difficult to determine if this represents intrinsic shape or is due to projection effects. Overall, the galaxy appears to be a relatively quiescent, evolved system.
