The galaxy presents as a spiral galaxy with a significant central bulge. While the image resolution is limited, a disk component is discernible. The galaxy exhibits spiral arm structure, though the arms are somewhat diffuse and not tightly wound. The color profile suggests the presence of both older stellar populations in the bulge and possibly regions of ongoing star formation within the disk. A relatively high luminosity implies a substantial mass. Overall, the galaxy appears to be a somewhat face-on spiral, presenting a moderate inclination relative to the line of sight. There may be some mild distortions or features that could be attributed to tidal interactions or minor mergers, though no clear merging partner is apparent. The light distribution suggests a fairly relaxed dynamical state, although further high resolution imaging and spectroscopic data would be needed to assess this accurately.
