The galaxy presents as a relatively smooth, elliptical-like structure. The light profile appears concentrated toward the center, with a gradual decrease in brightness moving outward. The primary color is yellowish-orange, suggesting a stellar population dominated by older, redder stars, with the possible presence of dust obscuration contributing to the redder hue. There is no strong evidence of spiral arms or prominent dust lanes. It appears the galaxy may be undergoing little to no active star formation. The round morphology suggests it may be relaxed and dynamically evolved, and does not currently show signs of any major merger activity.
