The galaxy presents as a fairly regular elliptical or lenticular type. It appears to be largely smooth in texture with a bright, concentrated central bulge, indicating a high degree of stellar population density in the core. Moving outward from the core, the galaxy's luminosity fades gradually. There is a hint of a disklike structure, though it is not a prominent feature. The light distribution suggests an older stellar population, likely dominated by redder stars, but with some evidence of ongoing or recent star formation appearing in the central region. No strong tidal features, dust lanes or other signs of recent major mergers are observed, although a minor disturbance is still possible given the subtle asymmetry. 
