The galaxy appears to be a single, moderately luminous object. Morphologically, it presents a relatively smooth structure, showing a subtle elongation. The color distribution across the galaxy seems to be subtly varied, with a slightly redder central region grading to a bluer hue in the outer regions. There is no obvious spiral structure or prominent disk features, and the overall texture suggests a relatively uniform distribution of light. There is no strong evidence of an ongoing major merger. The object is well-defined, with no obvious tidal tails or other features indicative of strong gravitational disturbance.
