This galaxy presents as a largely featureless, elliptical morphology. The light profile appears smooth and centrally concentrated, with a gradual decline in intensity from the core outwards. A slight elongation is observed, though the galaxy maintains a generally rounded appearance. The color indices suggest an older stellar population, with a redder hue dominating the central regions. The absence of prominent spiral arms, dust lanes, or bright, blue star-forming regions indicates a relatively quiescent star formation history, possibly representing a later stage in its evolutionary path. There is no strong indication of tidal disturbances or merging activity in the immediate vicinity. The galaxy is potentially at intermediate distance.
