The galaxy appears as a centrally concentrated, elliptical or lenticular-like structure. The core exhibits a yellowish-orange hue, indicative of an older stellar population dominated by redder stars. The outer regions of the galaxy display a fainter greenish-blue tint. This subtle colour variation suggests the presence of a younger, bluer stellar population in the outer regions, perhaps resulting from recent, yet limited, star formation activity. The overall morphology is generally smooth, with minimal evidence of spiral arms or significant dust lanes, with a slight, almost imperceptible disk shape. There is no indication of ongoing major mergers or significant tidal disturbances. It appears to be in a relatively quiescent state, with very low levels of star formation. The galaxy's shape is somewhere between round and cigar-shaped. Slight asymmetry is seen which could indicate a minor disturbance.
