The galaxy presents a largely smooth, elliptical morphology. The core exhibits a concentrated, bright yellowish hue, indicating a potentially older stellar population and negligible dust content. The overall shape appears somewhat rounded, with a slight elongation. No distinct spiral arm structures or prominent dust lanes are observed. There is little evidence of any major ongoing interaction or merging events, though subtle irregularities in the outer regions suggest minor past disturbances. The galaxy's color suggests a relatively low rate of current star formation.
