This galaxy presents as a centrally concentrated object with a noticeable, albeit somewhat amorphous, structure. Its overall morphology appears to be primarily smooth, with a lack of clearly defined spiral arms or a distinct bar. A subtle extension or feature seems present on one side, possibly indicating a minor disturbance or tidal interaction, although this could also be intrinsic to the galaxy's internal structure. The galaxy exhibits a gradual decline in luminosity from its core outwards. The central region displays a bright concentration, suggesting a possible active galactic nucleus or a dense stellar population.
