The galaxy presents as a compact, centrally concentrated object with a generally smooth appearance. Its light distribution suggests a somewhat elliptical morphology, tending toward being in between round and elongated. There is no obvious presence of distinct spiral arms or a well-defined disk structure. The galaxy exhibits a yellowish hue overall, which may indicate an older stellar population. No significant signs of major mergers or tidal disturbances are apparent in its immediate vicinity, though a very faint patch may indicate a minor interaction. The galaxy is moderately bright.
