The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly circular morphology, with the light appearing more condensed towards the center. While there are no clearly defined spiral arms or a prominent disk structure, the galaxy does not appear perfectly spherical, showing a slight elongation. There is a bright, concentrated central region that may indicate an active galactic nucleus or a dense stellar population. The galaxy appears primarily blue-white, with hints of redder colors at the edges, potentially indicating older stellar populations. There is no clear evidence of ongoing major mergers or tidal disturbances, though a slight asymmetry might suggest minor interaction or internal activity. Overall, the galaxy appears to be an early-type system that is not forming many stars, likely a lenticular or elliptical galaxy seen at a moderate distance.
