This galaxy presents as a somewhat elliptical, relatively compact structure. The central bulge exhibits a bright, concentrated luminosity, fading gradually towards the outer regions. The overall color profile leans towards a yellowish-white hue in the core, potentially indicating an older stellar population. Surrounding this central region, a less defined disk is visible, exhibiting a bluer tint, suggesting the presence of younger, hotter stars, indicating moderate star formation. The galaxy does not appear to display any prominent spiral arms, bars, or other major morphological features characteristic of grand design spirals. There is no readily apparent evidence of ongoing major mergers or significant tidal disturbances. Faint, diffuse regions extend outward from the main body of the galaxy, giving the impression of a weak halo structure. The overall impression is that of an intermediate galaxy type, possibly an early-type spiral or a lenticular galaxy undergoing mild star formation.
