The galaxy presents as a somewhat diffuse object, its light spread across a moderate area in the image. Its overall shape is predominantly elliptical, tending towards a flattened ellipsoid but not overtly cigar-shaped. The light distribution appears smooth, without obvious signs of significant spiral arm structure or large-scale irregularities. The color profile suggests a mixture of stellar populations. A redder hue dominates the central region, potentially indicative of older stars. This grades into bluer tones towards the outer edges, hinting at younger, hotter stars or regions of ongoing star formation. While not a strongly star-forming galaxy, the blue light suggests some level of recent or current star formation. There is no indication of any significant ongoing merger activity, the galaxy appears relatively undisturbed, with a small chance of being in a minor disturbance.
