The galaxy presents as an elliptical morphology with a high degree of central concentration. It is largely smooth in appearance, lacking prominent spiral arms or significant dust lanes. The shape is best described as being somewhere between round and cigar shaped. There is very little sign of interaction or merging activity visible. The galaxy exhibits a color gradient, appearing bluer at the core and gradually shifting towards redder hues in the outer regions. This may indicate an older stellar population dominating the galaxy’s overall light output, with some ongoing star formation localized near the center. The galaxy appears relatively isolated in this field of view.
