The galaxy presents as a well-defined elliptical shape, appearing largely smooth in texture. The core exhibits a concentrated, bright luminosity suggestive of a dense stellar population. A subtle color gradient is observed, with a slightly redder hue in the central region transitioning to a bluer tint within the surrounding outer halo. The galaxy exhibits a slight elongation suggesting a cigar shape. There is no visible evidence of spiral arms, dust lanes, or other prominent features typically associated with spiral galaxies. Overall, the galaxy appears to be an evolved system, potentially exhibiting minimal on-going star formation. No tidal tails or major disturbances are apparent, indicating that no recent major mergers have occurred.
