The galaxy presents as a relatively smooth, elliptical morphology, with a noticeable central bulge. The light distribution appears concentrated, exhibiting a gradual decline in brightness from the core outwards. The galaxy's color is predominantly yellowish-orange, suggesting an older stellar population. There is a slight elongation to the galaxy's shape; it is not perfectly spherical. Possible minor disturbances are indicated by slight asymmetries in the outer regions of the galaxy. There is no obvious evidence of spiral arm structure or a prominent disk component. The galaxy appears to be generally isolated with no clear signs of ongoing major mergers or interactions with nearby galaxies.
