The galaxy presents as a concentrated, somewhat elliptical entity. A dominant, smooth central bulge is visible, transitioning into a fainter, more diffuse surrounding structure. The galaxy appears relatively isolated, with no obvious signs of major interactions or significant tidal distortions. There may be a faint, almost imperceptible disk component. The color gradient indicates an aging stellar population, with a greater concentration of older, redder stars. The lack of pronounced spiral arms or bright star-forming regions suggests a relatively low star formation rate. The galaxy's overall structure leans towards that of an early-type galaxy, possibly an elliptical or lenticular.
