The galaxy presents a generally smooth, elliptical morphology. There is little evidence of distinct spiral arms or a prominent disk structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions.

The galaxy's color profile suggests a relatively evolved stellar population, with a tendency towards redder hues. This is indicative of older, lower-mass stars dominating the galaxy's luminosity. There are hints of subtle color variations within the galaxy, potentially reflecting differences in stellar populations or dust content.

Based on the morphology and color indices, this galaxy likely represents an elliptical galaxy with relatively low ongoing star formation. There is no apparent sign of any active galactic nucleus.
