The galaxy presents as a relatively smooth, elliptical morphology. Its overall shape is elongated, approaching a cigar-like form. The central region exhibits a concentrated, brighter luminosity, suggesting a prominent galactic nucleus. Moving outwards from the core, the luminosity gradually diminishes. There is some visual indication of slight disturbance in the outskirts, but no clear evidence of a major merger or tidal features. The galaxy displays a color gradient, transitioning from a yellowish hue in the center to a slightly bluer tint in the outer regions. This hints at a possible variation in stellar populations, with older stars concentrated in the core and a younger population contributing to the bluer light in the halo.
