This galaxy appears to be a relatively compact system, exhibiting a bright, concentrated core that dominates the overall luminosity. The core is surrounded by a diffuse halo with a slightly elliptical morphology. The isophotes are relatively smooth and regular, suggesting a lack of significant recent mergers or major disturbances. There is faint evidence of some low surface brightness features, which could be tidal debris or faint spiral arms, but the signal is weak. Overall, the galaxy presents as a relatively smooth, centrally concentrated system. There is the slight impression of a disk that cannot be confirmed with the given resolution.
