The galaxy presents a generally smooth and rounded morphology. There is a concentrated central bulge exhibiting a reddish hue, suggesting an older stellar population. Surrounding the bulge is a fainter, more diffuse disk with a slightly greenish tint, potentially indicating the presence of younger stars or ongoing star formation. No distinct spiral arm structures or prominent dust lanes are readily apparent. There are no obvious signs of a major merger or significant tidal disturbances in the galaxy's morphology. Overall, the galaxy appears to be a relatively undisturbed system.
