The galaxy presents as a relatively smooth, centralized light distribution with a slightly elongated morphology. The central region appears brighter and exhibits a yellowish-white hue, likely indicative of an older stellar population. Moving outwards from the center, the light gradually decreases in intensity. Faint bluish tones are visible in the outer regions, suggesting the presence of younger, hotter stars, though these regions lack distinct spiral arm structures. There is no evidence of significant tidal disturbances, major mergers or any obvious strong starburst activity. The galaxy has a relatively high degree of central concentration. Overall the galaxy appears as a relatively undisturbed system at moderate redshift.
