The galaxy appears as a relatively compact object with a smooth, centrally concentrated morphology. It exhibits a dominant, rounded central bulge, gradually fading into a less defined disk. There is an indication of some possible arm structure or features visible in the disk, though these appear somewhat diffuse and not highly structured. The galaxy's color profile suggests a mix of stellar populations, potentially with older, redder stars concentrated in the bulge region, and younger, bluer stars distributed throughout the disk. There is no obvious evidence of a significant merger event or major disturbance to the galaxy's overall form.
