The galaxy presents as a relatively smooth, centrally concentrated structure. The central region exhibits a bright, concentrated core, suggestive of an active galactic nucleus or a dense stellar population. A fainter, more diffuse halo surrounds the core. There may be signs of a possible disk or faint arm features extending away from the center but are not clear. The galaxy appears slightly elongated. Overall, there are no significant signs of a major ongoing merger, although subtle asymmetries may indicate a minor interaction or past disturbance. The color profile suggests the presence of both older stellar populations, contributing to the redder hues, and potentially some younger, bluer stars indicative of ongoing star formation, particularly in the outer regions.
