The galaxy presents as a centrally concentrated, elliptical morphology. Its color is a homogenous yellowish-orange, suggesting an older stellar population with a lack of significant ongoing star formation. The object appears largely smooth with no obvious spiral arm structure or dust lanes visible within this image resolution. There are no discernible tidal features or strong indications of recent merger activity, though subtle disturbances cannot be completely ruled out based on this single observation. The overall shape appears somewhat elongated but generally rounded rather than highly flattened. The effective radius is estimated to be relatively small.
