The galaxy presents as a relatively smooth, concentrated object with an apparent ellipticity. The main body of the galaxy exhibits a somewhat rounded morphology, though with a slight elongation. The color profile suggests a notable population of older stars, giving it a redder hue. There is evidence of blue light concentrations near its center. There is a slight disturbance in the galaxy's profile, a sign of a possible minor interaction or past merger event. The overall structure is not heavily disrupted, suggesting that any interactions were likely of relatively low impact.
