This galaxy presents as an elongated, cigar-shaped structure, consistent with an elliptical morphology viewed edge-on or a highly inclined spiral galaxy. The central region appears brighter and exhibits a yellowish hue, possibly indicating an older stellar population dominating the core.  Moving outwards from the core, the light fades gradually. There is a slight bluer tint at the extreme edges of the galaxy suggesting the presence of younger stars on the outer edges. The galaxy seems to be undisturbed, without any visible major mergers or tidal tails, though a possible minor disturbance cannot be fully ruled out.