The galaxy presents as an elongated, elliptical structure with a smooth, diffuse light distribution. The central region exhibits a higher concentration of light, suggesting a prominent galactic nucleus. The color profile is generally reddish-yellow, indicating a population of older stars, and suggesting a lower rate of ongoing star formation. There is little to no visible evidence of spiral arms or significant dust lanes. The overall morphology suggests a relatively quiescent galaxy, possibly an elliptical or lenticular type. There appear to be no signs of major mergers or significant tidal disturbances in the immediate vicinity.
