The galaxy presents a largely smooth, elliptical morphology, with a centrally concentrated luminosity profile. The core region appears bright and relatively uniform in color, suggesting an older stellar population dominating the light output. Moving outward from the core, the light gradually fades, and there is minimal evidence of spiral arm structures or distinct star-forming regions. The overall color index indicates a redder population, typical of galaxies where star formation has largely ceased, and older, redder stars dominate. There may be very minor disturbances present, but no clear signs of ongoing major merger activity or tidal distortions are apparent from its shape. The galaxy exhibits a fairly round appearance, without a highly elongated or disk-like structure.
