The galaxy presents as a well-defined elliptical structure with a smooth, diffuse light distribution. The central region exhibits a bright, concentrated core, indicative of a high stellar density. The color profile suggests a dominant population of older stars, as evidenced by the redder hues toward the central bulge, transitioning to slightly bluer colors in the outer regions. The overall shape is elongated, displaying an approximate axis ratio of 0.6, leaning more towards a cigar shape. There is little evidence of spiral arms or significant dust lanes. There are no significant tidal tails or obvious signs of recent major merger activity. The overall morphology suggests an evolved system with limited ongoing star formation. Faint disturbances are noted, but most likely there are no large scale interactions happening with other galaxies.
