The galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. Its color profile suggests a population dominated by older stars, evidenced by the reddish hue concentrated in the central region. The galaxy's shape is mostly round. There's no prominent dust lane or spiral arm structure visible. The galaxy appears to be fairly isolated, with no obvious signs of ongoing major merger activity. Based on these qualities, the galaxy likely resides further away in the universe.