The galaxy presents an elliptical morphology. The luminosity profile appears smooth and centrally concentrated, with a gradual decrease in surface brightness from the core outwards. The galaxy exhibits a yellowish hue, suggesting a stellar population dominated by older, redder stars. There is little evidence of spiral arms or prominent dust lanes. The galaxy's shape is elongated, appearing more cigar-shaped than circular. There are no obvious signs of recent or ongoing mergers or major disturbances in its structure, although a very subtle asymmetry cannot be ruled out. Based on the color and morphology, the galaxy is likely an early-type galaxy with relatively low levels of ongoing star formation.