The galaxy presents as a single, relatively smooth object with a concentrated central region. The morphology appears to be primarily spheroidal, exhibiting a gradual decrease in luminosity from the core outwards. There is a slight elongation to the galaxy's shape; it is not perfectly circular. Some faint, diffuse structures are visible extending from the main body of the galaxy, though these are not clearly defined spiral arms or tidal tails. These faint structures appear slightly bluer in color than the central bulge, implying the presence of younger stellar populations. The dominant color of the galaxy appears to be yellow to reddish. This suggests an older stellar population. The galaxy does not display any prominent dust lanes or signs of active star formation in the core. 
