The object presents as a relatively small, centralized galaxy. The overall color profile leans towards the green end of the spectrum, suggesting a population of younger, hotter stars and/or significant ongoing star formation. The central region exhibits a bright, concentrated luminosity, likely indicating the presence of a dense stellar population or perhaps an active galactic nucleus. The morphology appears somewhat disturbed. There is a clear asymmetry in the galactic disc, potentially suggestive of tidal interactions with another galaxy. Patches of magenta appear in the outer edges of the disc which could suggest regions of elevated activity.
