The galaxy presents as a single, relatively smooth and rounded object with a concentrated central bulge, characteristic of an elliptical morphology. The galaxy exhibits a yellowish-orange color, suggestive of an older stellar population with minimal ongoing star formation. It appears to be potentially interacting or merging, as the general form looks like there are two cores. Though no distinct tidal tails are observed in this image, the morphology appears disturbed, potentially hinting at a merger event. It would be useful to analyze spectra for emission lines to determine the current state of the galaxy.
