The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light profile appears to peak sharply at the center, suggesting a prominent bulge component. The overall color is yellowish, indicative of an older stellar population and suppressed star formation activity. There is little evidence of spiral arm structures or prominent dust lanes. A slight elongation is perceptible, hinting at a possible elliptical shape, although the roundness is notable. No signs of major merger activity or significant tidal disturbances are apparent in the immediate vicinity of the galaxy. There may be a slight hint of a disk, but it is not as prominent as the bulge component. The galaxy appears relatively isolated based on the absence of close companions or interactions.