The galaxy presents a generally smooth morphology, with a centrally concentrated light profile. The object exhibits a slightly elliptical shape, falling somewhere between perfectly round and more elongated. There is little to no evidence of spiral arms or a distinct disk structure. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances, exhibiting an unperturbed structure. The color profile suggests a population dominated by older stars, exhibiting a redder hue at the core with a slight bluing towards the outer edges. Overall, the galaxy appears as a relatively undisturbed, evolved system.
