The galaxy presents an overall smooth, elliptical morphology, with a notable elongation along its major axis. Its color profile appears relatively uniform, with a dominant yellowish-orange hue, suggesting a population of older stars and/or a significant dust component. There is no strong evidence of spiral arm structure or prominent star-forming regions. The galaxy's light profile appears concentrated towards the center, indicating a dense stellar nucleus. There is a subtle suggestion of some minor tidal disturbances or faint features extending from the galaxy's main body, especially along the major axis, although this is uncertain. The overall appearance points to a passively evolving system, though deeper observations would be necessary to confirm this.
