The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellowish hue. This suggests an older stellar population dominating the core. The overall shape is elongated, approaching a cigar-like appearance. There's a subtle fading of color intensity moving outwards from the central region, transitioning from yellow to a faint reddish tint in the outer edges, implying a possible presence of dust or variations in stellar populations across the galaxy's extent. There is no definitive spiral structure visible; it appears to be a relatively evolved system, undisturbed by any major mergers or interactions in its recent history.
