The galaxy appears to be a relatively smooth, elliptical type, exhibiting a somewhat elongated morphology rather than a perfect sphere. There is a noticeable concentration of light towards the center, suggesting a prominent galactic nucleus. The overall color gradient transitions from a yellowish hue in the core to a slightly redder tone in the outer regions, potentially indicative of older stellar populations in the outskirts. There is some slight visual disturbance that may indicate a minor interaction or tidal effect. Although there is not much evidence of distinct spiral arms or significant dust lanes, the presence of a faint disk component cannot be ruled out.
