The galaxy presents as a relatively bright, disk-shaped structure with a notable central bulge. The bulge appears largely homogenous and exhibits a yellow-white hue, suggesting an older stellar population. The disk is oriented at a shallow angle relative to our line of sight. The disk demonstrates a mottled texture, indicating a non-uniform distribution of stars and dust. There appears to be no strong evidence of spiral arm structure from the image. The overall color profile suggests a higher concentration of older stars throughout the galaxy, with a limited presence of bluer, younger stars. There is very slight evidence of tidal disturbances in the image. There is likely very little active star formation occurring in this galaxy.
