The galaxy presents as a well-defined elliptical morphology, exhibiting a smooth, concentrated light profile. The central region is a bright, yellowish hue, suggesting a population of older stars. The galaxy appears elongated, with a cigar-like shape. There is a hint of a subtle color gradient from the center outwards, with the outer regions displaying a slightly bluer tint. This may indicate ongoing, albeit low-level, star formation in the galaxy's outskirts. No distinct spiral arms or prominent dust lanes are visible. There are no obvious signs of any major mergers or tidal disturbances affecting the galaxy's structure, though there might be very minor disturbances.
