The galaxy presents as a single, relatively smooth object with an elliptical morphology. It appears mostly featureless, lacking any distinct spiral arms or prominent dust lanes. The light is centrally concentrated with a gradual decrease in intensity toward the outer edges. The color profile indicates a higher concentration of older stellar populations, as evidenced by the reddish-yellow hue. There is little indication of active star formation based on the overall color. The galaxy exhibits a mild deviation from perfect circularity, appearing slightly elongated, but is not considered cigar shaped. There are no visual signs of any major merging events or significant tidal disturbances in the immediate vicinity. Any minor disturbances would require closer inspection in higher resolution. Overall, the galaxy appears to be a relatively evolved, quiescent system, consistent with an early-type morphology.
