The galaxy presents a smooth, elliptical morphology. Its light profile appears concentrated, exhibiting a bright, yellowish core. The overall shape is generally rounded with a slight elongation suggesting it leans slightly to a cigar shape but mostly falls between the round and cigar shaped classification. There are no prominent spiral arms, dust lanes, or other obvious features indicative of active star formation regions. Color gradients suggest the presence of an older stellar population dominating the light output. There is no indication of any major merging events, though minor disturbances cannot be completely ruled out. The galaxy appears to be fairly isolated and undisturbed.
