The galaxy appears to be an elliptical type, displaying a relatively smooth, featureless morphology overall. It exhibits a moderate elongation, tending towards a more in-between roundness than a fully circular shape. There are indications of a possible disturbance or interaction, as the galaxy lacks the pristine symmetry often associated with isolated ellipticals. While no distinct tidal tails or bridges are immediately apparent in this image, the overall structure suggests some level of past or ongoing gravitational interaction. The color profile reveals an older stellar population, as evidenced by the redder hues compared to bluer, star-forming galaxies.
