The galaxy presents as a slightly elongated, somewhat spindle-shaped structure. The central region exhibits a concentrated luminosity, appearing yellowish-white, indicative of an older stellar population. Moving outwards from the core, a gradual decrease in brightness is observed, with a subtle color shift towards a blue-green hue. This could represent younger stars in the outer regions. The overall morphology suggests a relatively smooth texture with minimal evidence of distinct spiral arm structures. There are no obvious signs of significant tidal distortions or ongoing major mergers. The galaxy appears to be in a relatively quiescent state, with perhaps a modest amount of star formation occurring in the outer disk.
