The galaxy presents a predominantly smooth morphology, with an approximately circular shape. The central region exhibits a concentrated luminosity, displaying a yellowish-orange hue, suggestive of an older stellar population. Surrounding the core, there appears to be a fainter, more diffuse halo characterized by a slightly bluer color, possibly indicating the presence of some younger stars or ongoing star formation. There is little evidence of spiral arms or a distinct disk structure. The overall structure appears relatively undisturbed, without significant signs of tidal interactions or major merging events.
