The galaxy presents a generally smooth, elliptical morphology. The central bulge is prominent, exhibiting a concentrated luminosity profile with a yellowish hue, indicating an older stellar population. A faint disk component appears to be present, although it is not clearly defined, showing some bluer regions which may be indications of star formation. The overall color of the galaxy suggests a redder spectral energy distribution, with the core region appearing significantly redder compared to the outer regions. The galaxy exhibits some slight disturbances that may be due to minor interactions with other galaxies.
