The galaxy appears to be an elliptical type, exhibiting a smooth and relatively featureless morphology. Its shape is somewhat elongated, resembling a cigar. A bright central bulge dominates the galaxy's structure, with light intensity gradually decreasing towards the outer regions. The color profile suggests a population of older stars, indicated by the yellowish-orange hue. There is no visible evidence of significant spiral arm structure or ongoing major merging activity. Faint wisps of diffuse light extend beyond the central region, possibly indicating a tenuous halo. The galaxy appears generally undisturbed, displaying a settled and evolved state.
