The galaxy presents as a somewhat elliptical, smoothed structure. A bright central bulge is clearly visible. The overall color distribution is a gradient. The core displays a yellowish-white appearance, suggesting an older stellar population. Progressing outwards, the disk exhibits a bluer hue, possibly indicating areas of ongoing star formation. No distinct spiral arms are apparent within the visible structure. There is a slight asymmetry observed, possibly hinting at a minor tidal interaction or internal disturbance within the galaxy. The majority of the light appears centrally concentrated.
