The galaxy presents as a moderately bright, elliptical or lenticular system, exhibiting a smooth, diffuse light distribution across its main body. There's a suggestion of a central bulge, slightly brighter and more concentrated than the surrounding halo, and a disk component is likely present. The galaxy's major axis appears significantly longer than its minor axis, giving it a somewhat elongated, cigar-like shape. There's a possible minor disturbance in its morphology, although a major merger seems unlikely. Star formation rates appear subdued. The color index suggests a population of older stars. Overall, the galaxy appears to be an evolved system approaching quiescence.
