This galaxy exhibits a generally smooth morphology, with a dominant spheroidal component. It appears elongated, suggesting a possible classification as an elliptical galaxy, possibly of type E4-E7 depending on the precise axis ratio. The central region displays a pronounced concentration of light, with a reddish hue, potentially indicative of an older stellar population and/or dust obscuration. Moving outwards from the core, there is a noticeable transition to bluer colors in the outer regions. This suggests the presence of younger stars and/or ongoing star formation in the galactic disk. There is no clear evidence of spiral arm structure or significant tidal disturbances, supporting the classification as a relatively undisturbed galaxy. Overall, this appears to be a galaxy undergoing some ongoing star formation in the outer disk regions, while the central core is dominated by an older stellar population.
