The galaxy appears as a moderately bright, centrally concentrated object. Its morphology is primarily smooth, lacking defined spiral arms or a prominent disk structure. The overall shape is roughly elliptical, though it leans towards being in-between elliptical and round. There is a hint of a flattened appearance but it is not particularly elongated.

The color profile suggests a relatively evolved stellar population, with a yellowish-white core indicative of older stars and potentially less active star formation. Faint hints of blue tinge at the edges could be evidence of some ongoing, though limited, star formation activity. There may be a very slight disturbance within the galaxy's structure, but any indication of a merger is subtle.
