The galaxy appears as a somewhat elliptical, centrally concentrated object with a smooth, diffuse light profile. The galaxy exhibits a yellowish-white hue in its central region, suggesting an older stellar population. The radial color gradient appears subtle, transitioning from a slightly more yellow core to a marginally redder halo. The lack of distinct features indicates a relatively quiescent state. There is no clear evidence of spiral arms or dust lanes. The overall appearance suggests an elliptical galaxy with a considerable mass. There are minor disturbances appearing on the edges of the galaxy that suggest a small chance of the galaxy going through a minor merger. The galaxy appears to be a transitional form somewhere between an elliptical and a cigar shaped morphology. The galaxy has a low star formation rate.
