The observed galaxy presents as a centrally concentrated object, appearing largely smooth in structure. It exhibits a generally elliptical morphology, with a suggestion of moderate roundness rather than a highly elongated or cigar-like form. There is an indication of some interaction or disturbance, which could be a minor interaction with a small nearby object. The core of the galaxy is more luminous, indicative of a higher stellar density or active galactic nucleus. The color appears predominantly yellow/orange which suggest a population dominated by older stars and a relatively low rate of on-going star formation. 
