The galaxy presents as a relatively compact object, exhibiting a smooth and largely featureless morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The overall shape is somewhat elliptical, leaning towards an oblate form rather than a highly elongated or cigar-like structure. There is no readily apparent spiral arm structure or significant dust lane obscuration. No signs of major mergers or tidal disturbances are immediately visible. The galaxy appears relatively isolated. The central region appears brighter and more bluish in color, suggestive of a population of younger, hotter stars or active galactic nuclei. Overall, the galaxy's characteristics align with those of an elliptical or lenticular galaxy, exhibiting an apparent lack of significant ongoing star formation outside of the central region.
