The galaxy presents as a generally smooth, elliptical-shaped structure with a bright, concentrated central bulge. The color profile exhibits a gradient, transitioning from a yellowish-white core to a slightly redder outer halo. There is minimal evidence of distinct spiral arms or prominent dust lanes within the resolution of the image. The galaxy exhibits a moderate degree of ellipticity. There appears to be minimal morphological evidence of recent or ongoing major mergers, however, there is some indication of minor disturbances. Based on its color and smooth morphology, the galaxy likely consists of an older stellar population with a low star formation rate.
