The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution is centrally concentrated, with a gradual decrease in luminosity outward. The core exhibits a yellowish-red hue, suggesting an older stellar population. The overall form suggests a lack of significant recent merging activity or major disturbances. There are no prominent spiral arms or intricate dust lanes visible. The galaxy does not appear to be actively star-forming in large quantities, based on its redder color, but has a small amount of blue light, suggesting some star formation may be occurring. Overall, the galaxy is characterized by a generally smooth appearance, dominated by an older stellar population with a concentrated central bulge and has an intermediate mass with a moderate rate of star formation. 
