The galaxy presents as a moderately small object with an elliptical morphology. A smooth light distribution is observed. The galaxy's core region displays a relatively concentrated appearance. The general hue suggests a redder color profile. There is an indication of a potential minor disturbance or interaction in the form of a slight asymmetry or lopsidedness in the galactic structure, possibly related to a minor merging event. The overall appearance implies a galaxy that is likely an elliptical galaxy with some evidence of past or ongoing interaction.
