The galaxy presents as an elongated, elliptical morphology with a smooth light distribution. The central region exhibits a concentrated, bright core, suggesting a high stellar density. The color profile transitions from a yellowish-white hue at the core, indicative of an older stellar population, to a slightly bluer tinge in the outer regions, potentially signaling more recent star formation. There is no discernible spiral arm structure or significant dust lane obscuration visible in this image. The overall appearance suggests a relatively evolved system, with a small degree of ongoing star formation at the edges of the galactic disk. There is no obvious indication of active galactic nuclei activity or tidal disruption in this image.
