The galaxy presents as an elliptical morphology, viewed at an oblique angle. It exhibits a smooth luminosity profile, with a centrally concentrated bulge that fades gradually into the outer regions. The galaxy appears more elongated than circular. There is an observed color gradient, with the core exhibiting a yellowish to reddish hue, potentially indicative of an older stellar population or dust obscuration. The outer regions are bluer, possibly indicating ongoing star formation, though it is not concentrated in spiral arms. There appears to be some minor structural disturbance on the left side of the image, potentially indicative of a minor merger or tidal interaction. The galaxy shows a small amount of ongoing star formation.
