The galaxy presents a generally elliptical morphology, with a smooth appearance across its main body. A bright central bulge is observed, exhibiting a yellowish-white hue suggestive of an older stellar population dominating the core. The galaxy's disk appears moderately inclined relative to the observer's line of sight. Hints of bluer regions are present within the disk, possibly indicating areas of more recent star formation. There are suggestions of minor tidal disturbances or asymmetries in the outer regions of the galaxy, most visible on the left, possibly indicative of past or ongoing interactions with another galaxy. However, no major distortions or signs of a significant merger event are immediately apparent.
