The galaxy presents as a single, primarily smooth object. It exhibits an elliptical morphology, with a shape tending towards but not fully cigar-shaped. There are no obvious indications of a spiral structure or distinct disk component. The galaxy appears to be dominated by a central bulge, with a radial gradient from a bright, concentrated core outward to fainter, more diffuse edges. The color profile is generally consistent, with a yellowish hue that suggests a stellar population dominated by older, redder stars. There is no pronounced evidence of ongoing major mergers or tidal disturbances, and no apparent dust lanes or patchy star formation regions. Minor asymmetrical features might indicate some subtle past interaction. Overall, the galaxy appears to be a relatively evolved, undisturbed system.
