The galaxy appears to be elliptical in morphology, with a smooth light distribution. The galaxy's central region is more concentrated and brighter, with a yellowish hue, which suggests an older stellar population. Moving outward from the core, the light becomes more diffuse, forming a halo-like structure. The overall shape is elongated, displaying a cigar-like form. There are no apparent signs of spiral arms or prominent dust lanes. No signs of interaction or ongoing mergers are visible.
