The galaxy appears to be a relatively smooth system, with a generally elliptical morphology. It displays a notable central bulge, which dominates the overall light profile. The color index indicates a redder hue, suggesting a population of older stars, and reduced star formation, particularly near the center. The galaxy shows some evidence of potential tidal disturbances, with some distortions visible, possibly due to gravitational interactions with another system. At least one apparent companion galaxy is detected near the main galaxy, suggesting a possible merger event in its past, or in the future. The galaxy exhibits a moderate level of roundness, showing that it is not highly elongated. Overall, the galaxy seems to be in transition, possibly from a spiral to an elliptical galaxy, as it is exhibiting signs of interaction and disturbance, along with having a smooth profile overall.
