The galaxy presents as a relatively smooth, elongated structure. The central bulge is prominent, exhibiting a concentrated luminosity gradient that fades gradually towards the outer regions. The morphology appears to be elliptical, with the galaxy displaying a lack of distinct spiral arms or prominent dust lanes. There is a subtle color gradient observable, with the central bulge showing a slightly yellower hue compared to the bluer, less intensely luminous outskirts. The overall appearance suggests a system dominated by older stellar populations with a possible, though not distinct, disk. The shape is not perfectly round, but deviates towards an elongated, cigar-like form. There's no immediately apparent evidence of significant ongoing merger activity or major disturbances in the galaxy's structure.
