The galaxy presents as a lenticular or early-type spiral, seen nearly edge-on. The central bulge exhibits a smooth, concentrated luminosity profile, appearing yellowish in color, suggestive of an older stellar population. A faint, flattened disk is visible, extending beyond the bulge. The disk's color shifts towards a bluer hue, potentially indicating the presence of younger, hotter stars, though the overall low surface brightness of the disk implies a relatively low star formation rate. There are no distinct spiral arms visible, and the disk appears largely featureless. The galaxy displays a slightly elongated morphology, with an axial ratio greater than 2:1. There is no strong evidence of any major ongoing merger activity, although subtle asymmetries or minor tidal disturbances cannot be ruled out based on the image alone. Overall, the galaxy appears to be a relatively quiescent system.
