The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a bright, unresolved core which suggests a high stellar density, likely dominated by an older stellar population. Moving outwards from the core, the light gradually diffuses with no obvious spiral arm structures or dust lanes visible. The overall color is generally consistent with a galaxy undergoing relatively low levels of star formation, as indicated by the redder hue. There is a hint of a slightly bluer color in the outer regions which suggests there are younger, bluer stars. The galaxy is not perfectly spherical, but displays only a slight deviation towards a cigar shape. There is no apparent major merger activity or significant tidal disturbance, though the galaxy is not perfectly isolated, showing minor disturbances.
