The galaxy presents a generally smooth and rounded appearance, with little evidence of spiral arms or significant disk structure. Its light profile suggests a concentrated central region that gradually fades outwards. There is a color gradient, with a yellowish-white core transitioning to redder hues in the outer regions. This color change might indicate a different stellar population in the outer regions or a differential dust extinction. Based on these features, this galaxy is likely an elliptical galaxy, possibly with a small amount of ongoing star formation.
