The galaxy presents as a moderately bright, elliptical structure, with a concentrated central bulge. The light distribution appears smooth and diffuse, lacking distinct spiral arms or prominent features associated with active star formation. The color profile suggests a population of older stars dominating the galaxy's composition, exhibiting a yellowish-orange hue. The shape is elongated, with a notable difference between its major and minor axes, indicating a relatively high inclination with respect to our line of sight. There are no obvious signs of recent major mergers or tidal disturbances, although a subtle asymmetry in the outer regions could suggest minor past interactions.
