The galaxy presents as a largely smooth, featureless object. It exhibits a generally elliptical morphology with a relatively high degree of elongation, appearing cigar-shaped. A central bulge is present, exhibiting a significantly brighter intensity compared to the surrounding galactic disc. The overall color profile is dominated by warmer tones, trending towards yellow and red, suggesting a population of older stars and a lower rate of on-going star formation activity. There is no apparent evidence of active galactic nuclei activity from the color profile. No significant signs of tidal disturbances or ongoing mergers are apparent.
