The galaxy presents as a relatively compact object with a flattened spheroidal shape. There is a concentration of light toward the central region, which appears more prominent than the outer edges. The galaxy exhibits a smooth morphology, with no obvious spiral arm structures or prominent dust lanes visible at this resolution. There is an apparent slight distortion in the overall shape suggesting possible past or ongoing interaction. The color of the galaxy appears relatively uniform and indicates an older stellar population. There is some indication of ongoing, but relatively low, star formation within the galaxy.
