The galaxy appears as a slightly elongated, unresolved object. Its color profile exhibits a concentration of reddish-orange hues in the central region, suggesting a possible population of older stars dominating the core. A faint, diffuse greenish halo surrounds the core, possibly indicating regions of lower metallicity stars, or some on-going star formation activity. The lack of distinct morphological features suggests a relatively smooth distribution of stellar populations. There is no obvious evidence of spiral arms or a bar structure. It appears as a mostly isolated galaxy, with no visual signs of major tidal disturbances or ongoing mergers.
