The galaxy presents a relatively smooth and rounded appearance, exhibiting a concentrated central bulge. Its light profile suggests a well-defined core that gradually fades outward. The galaxy's color is predominantly yellowish, indicating a population of older stars with lower rates of star formation and relatively low specific star formation rate. There is little evidence of spiral arms or significant disk features, which, with the smooth structure, may indicate this is an elliptical galaxy or lenticular galaxy. Faint hints of disturbed light suggest a minor interaction with another object, though no clear merger features are present. The mass of the galaxy is substantial. The overall morphology indicates it is a mature galaxy with a stable structure.
