The galaxy appears as a centrally concentrated, luminous object. It is elliptical in shape, though tending toward a more disk-like form. There's a central bulge, though not particularly prominent, with a diffuse glow around it. The galaxy exhibits a color gradient, shifting from a yellowish core to a redder hue in its outer regions. No distinct spiral arms or dust lanes are visible; instead, a relatively smooth morphology is observed. There are no significant signs of tidal disturbances or ongoing major mergers. The galaxy is likely to have a moderately high stellar mass and a relatively low star formation rate.
