The galaxy appears as an elliptical or lenticular system, displaying a smooth, centrally concentrated luminosity profile. Its shape is elongated, exhibiting a cigar-like morphology. There's a clear absence of prominent spiral arms or a well-defined disk structure. The core of the galaxy presents a bright, concentrated region, indicative of a possible galactic bulge. The overall color profile suggests an older stellar population, with a redder hue dominating. There are no obvious signs of major mergers or significant tidal disturbances, although a subtle asymmetry might suggest a minor interaction in its past.
