The galaxy presents a primarily smooth, elliptical morphology. Its central region exhibits a concentrated luminosity with a redder hue, suggesting an older stellar population. The outer regions display a faint, disk-like structure with hints of bluer light, implying the presence of some younger stars and ongoing star formation, albeit at a relatively low rate. Overall, the galaxy appears to be in a relatively undisturbed state, with no major signs of tidal interactions or mergers. The shape appears somewhat flattened, exhibiting a deviation from a perfectly circular form, leaning towards an intermediate classification between round and elongated.
