The galaxy presents as a relatively small, lenticular shaped object. Its light profile appears smooth, without prominent spiral arm structures or significant dust lane obscuration. The core region of the galaxy seems slightly brighter and more condensed than the outer regions. There is a gradual decrease in luminosity from the center toward the edges, indicating a lack of significant star forming regions contributing to the overall light. The galaxy exhibits a blue hue. The outer edges do not appear sharp, but rather diffuse, suggesting a halo of older stars or a gradual transition into the intergalactic medium. There's no obvious signs of tidal disruption or interaction with nearby galaxies. Overall, this appears to be a relatively undisturbed galaxy in its later stages of evolution.
