The galaxy presents an overall smooth, elliptical morphology, with an apparent lack of distinct spiral arm structure. The galaxy's light profile appears centrally concentrated. The major axis is oriented approximately horizontally within the field of view, exhibiting a slightly elongated shape, but leans closer to round than cigar shaped. The galaxy's color suggests a population of older stars, or significant dust content, as indicated by the redder hue in the 'r' and 'z' bands relative to the 'g' band. There are some subtle irregularities in the light distribution that *may* suggest minor tidal interactions or internal disturbances, but these are not pronounced. Overall, the galaxy appears relatively undisturbed.
