The galaxy presents as a largely smooth object with a concentrated central bulge. There is a subtle extension of light extending from the central region, potentially indicative of a faint disk or arm structures, though these are poorly defined. The color profile suggests an older stellar population, dominated by redder wavelengths. The galaxy exhibits a slightly elliptical shape, with an intermediate axis ratio. There are no obvious signs of active merging or tidal disturbances within the immediate vicinity of the galaxy. The galaxy appears relatively isolated based on the field of view.
