The galaxy presents as an elliptical morphology. The central region exhibits a concentrated luminosity, appearing relatively smooth and unstructured, potentially indicating an older stellar population. A faint, diffuse disk component is also present, with a bluer hue, possibly representing ongoing or recent star formation activity. The galaxy's overall structure is moderately disturbed. There may be very faint signs of tidal interactions or a past merger event, with a slight asymmetry in the outer regions, but there is no current merging activity. The galaxy exhibits a moderate redshift. The angular size appears small, suggesting a significant distance.
