The galaxy presents a largely smooth and elliptical morphology. Its core is characterized by a bright, concentrated luminosity, suggesting a high stellar density. The overall color appears to be a yellowish-orange, potentially indicative of an older stellar population with fewer ongoing star formation processes and a higher abundance of redder stars. The isophotes are relatively regular, exhibiting little evidence of significant tidal disturbances or recent merger events. A subtle extension of light is visible beyond the central bulge, implying the presence of a more diffuse stellar halo or an extended disk component. Based on the observed characteristics, this galaxy could be classified as an early-type galaxy with a substantial mass and a moderate amount of past star formation activity.
