The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated, bright central bulge. The color gradient transitions from a yellowish-orange hue at the core to a slightly redder tint in the outer regions. There's minimal evidence of distinct spiral arms or prominent dust lanes, suggesting an older stellar population and a lower rate of ongoing star formation. The overall shape appears largely undisturbed, indicating a lack of recent major merger activity. Minor irregularities or asymmetries are not readily apparent within the resolution limits of the image, and it doesn't seem to be undergoing any major interactions with neighboring galaxies. The galaxy presents with a very round shape.
