The galaxy presents a somewhat elliptical morphology, appearing as an elongated, cigar-shaped structure. The light distribution suggests a concentration towards the center, indicating a prominent galactic bulge. The galaxy exhibits a smooth overall appearance, with no readily discernible spiral arms or significant dust lanes. The color profile indicates a predominantly older stellar population, emitting more light in the redder wavelengths. The observed shape might imply an ongoing or past merger event, though there aren't any clear tidal tails or obvious signs of major disturbance. It appears to be a relatively massive system. The absence of strong blue light suggests a relatively low rate of ongoing star formation.
