The galaxy presents as a roughly elliptical structure with a bright, concentrated central bulge. The galaxy displays a smooth overall appearance, with little evidence of significant spiral arm structure or irregular features. The color profile suggests an older stellar population, particularly in the central bulge, which exhibits a yellowish-white hue, indicating the presence of evolved stars. A faint, bluer disk component may be present, subtly extending from the central region. There is no clear indication of ongoing major merging activity or significant tidal distortions. However, a few subtle asymmetries or minor disturbances may be present in the faint outer regions.
