The galaxy presents a generally smooth morphology. It appears elliptical in shape, with a bright, concentrated central bulge that transitions smoothly into a fainter, more diffuse halo. The halo exhibits a slight elongation, suggesting it is not perfectly spherical. Color gradients are subtle, with a yellowish hue dominating the central region, possibly indicative of an older stellar population. Fainter blueish tints appear asymmetrically in the periphery of the galaxy, suggesting the presence of localized regions with ongoing star formation. There appears to be no clear evidence of spiral arm structure or significant dust lanes within the galaxy. Overall, the galaxy shows little evidence of major disturbances, although there is a slight unevenness to the left of the galaxy, possibly resulting from a minor interaction.
