The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. Its color appears yellowish-orange, suggesting a stellar population dominated by older, redder stars, and potentially indicating relatively low levels of ongoing star formation. The galaxy's shape is somewhat elongated, leaning toward an "in-between" roundness. There are no readily apparent signs of spiral arms, dust lanes, or tidal disturbances. It does not visually appear to be undergoing a major merging event, with no extreme asymmetries or morphological peculiarities.
