The galaxy appears to be a relatively smooth, elliptical or lenticular type. It displays a concentrated central bulge, which appears yellowish, suggesting an older stellar population. The isophotes are generally circular, with only a very slight deviation from perfect roundness. The galaxy exhibits a bluer color at larger radii, indicating a possible presence of younger stars in the outer regions. There is no strong evidence of spiral arm structure or significant dust lanes, which is in agreement with a classification towards the elliptical end of the Hubble sequence. No obvious signs of major mergers or tidal disturbances are observed, although there may be some minor irregularities suggesting potential past interactions. The overall structure is relatively simple and well-defined.
