The galaxy presents a generally smooth morphology, with a centrally concentrated luminosity profile. It appears elliptical in shape, displaying a relatively high degree of symmetry. The core region exhibits a bright, somewhat diffuse glow, transitioning to a bluer hue in the outer regions. The light from the core suggests an older stellar population, while the outer regions might contain younger, bluer stars, or possibly exhibit weak active star formation. There is no obvious evidence of spiral arm structure or a prominent dust lane, but there may be subtle disturbances suggesting minor gravitational interactions or past merger events. The overall color is consistent with a mature galaxy, showing a shift toward the redder end of the spectrum, although some bluer regions may indicate on-going star formation.
