The galaxy presents a generally elliptical morphology, although some irregularity is apparent. The object exhibits a smooth appearance, with no immediately obvious spiral arm structures or a prominent central bar. There is evidence of a merging or disturbed system. The light distribution is somewhat concentrated, with a noticeable decrease in surface brightness moving outwards from the center. The galaxy's color profile indicates a redder hue, especially in the central regions, likely due to an older stellar population or significant dust obscuration. Overall, it appears to be a relatively quiescent galaxy.
