The galaxy presents as a centrally concentrated object with a relatively smooth appearance. Its morphology suggests a spheroid-like shape, appearing more "in between" round and elongated, with no prominent spiral arms or a well-defined disk component readily discernible. The core region exhibits a bright, yellowish-white hue, which could be indicative of an older stellar population or a significant bulge. The outer regions of the galaxy fade gradually into the background sky, showing hints of a faint, extended halo. There appears to be very minimal signs of any major disturbances or merging events within the galaxy's structure. The overall color profile suggests it is dominated by evolved stars, potentially with a low ongoing star formation rate.
