The galaxy presents as a slightly elongated spheroid with a noticeable central bulge exhibiting a concentrated luminosity. There is evidence of a disk, but it is not well defined. The galaxy exhibits a generally smooth texture, with the majority of its light distributed relatively evenly across its surface, gradually decreasing in intensity away from the central bulge. The light is yellowish-white, suggesting a population of older stars, with a slight redder tint in the outer regions. The morphology suggests a moderate mass galaxy with a relatively low star formation rate. There is no clear evidence of a major merger or significant tidal disturbances, however, there is another nearby galaxy that may be interacting.
