The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The light distribution appears centrally condensed, transitioning smoothly outwards without distinct features like spiral arms or a prominent bar. A slight elongation is noticeable, though the object is mostly round. A faint arc-like feature is visible, possibly indicating a gravitational lens effect or tidal stream, although the resolution is not high enough to determine its origin with certainty. The galaxy's overall color appears to be slightly yellowish, suggesting an older stellar population and relatively low levels of ongoing star formation. There is no obvious evidence of a major ongoing merger, although subtle disturbances cannot be ruled out.
