The galaxy presents as a somewhat elongated, disk-like structure. There appears to be a central bulge, which is the brightest and most concentrated region. This bulge transitions smoothly into a fainter, more diffuse disk. The galaxy exhibits a generally smooth appearance, lacking prominent spiral arms or distinct star-forming regions that are resolvable at this resolution. The overall color suggests the presence of both older stellar populations in the central region, which contributes to the redder hues, and some younger, bluer stars in the outer regions. There are no strong indications of tidal disturbances or ongoing mergers in the image. The galaxy seems relatively undisturbed and appears as an isolated system.
