The galaxy presents as a roughly elliptical system, appearing largely smooth in texture, with minimal evidence of spiral arm structure or significant dust lanes. The color profile indicates a dominant population of older stars, contributing to its reddish hue. The galaxy demonstrates a concentrated central bulge, with a gradual decrease in luminosity outwards. The overall morphology suggests it is an early-type galaxy, possibly an elliptical or lenticular galaxy nearing quiescence. There is no obvious central active galactic nucleus or signs of ongoing major mergers. The system exhibits a moderate level of star formation.

