The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The galaxy exhibits a yellowish-orange hue, suggesting an older stellar population with lower star formation activity. Its morphology is predominantly smooth with no apparent spiral arm structure or significant dust lanes. The overall shape is fairly round, showing minimal signs of disturbance or tidal interactions. There are no visible signs of recent or ongoing mergers, and the galaxy appears to be isolated. The galaxy presents a distinct color gradient, transitioning to redder hues toward the central regions, implying a possible concentration of older, redder stars.