The galaxy presents a largely smooth and rounded morphology. It appears as a single, fairly homogenous structure with a bright, concentrated core. There's a subtle color gradient, with the central region exhibiting a bluer hue that gradually fades into a redder color towards the outer edges. No distinct spiral arms or bar structures are discernible. The overall appearance suggests a galaxy with minimal recent or ongoing major star formation activity. The light is relatively even, indicating a well-mixed stellar population, possibly dominated by older stars. There is no evidence of tidal disturbances or close companions suggesting a recent merger event. Based on its physical size and brightness, it would be classified as a dwarf galaxy.