The galaxy presents as an elongated, somewhat cigar-shaped structure, exhibiting a generally smooth appearance. The central region is distinctly brighter and displays a yellowish-orange hue, indicative of an older stellar population. The outer regions of the galaxy appear fainter and more diffuse, with a subtle transition in color towards a slightly bluer shade, potentially suggesting the presence of some younger stars, although the overall star formation rate appears to be relatively low. There is no prominent spiral structure or any distinct disk component visible. No major signs of tidal disruption or interaction with other galaxies are apparent. The galaxy's morphology is largely undisturbed.
