The galaxy presents a predominantly smooth morphology, suggesting it is likely an early-type galaxy. Its shape is moderately elliptical, appearing somewhat elongated rather than perfectly spherical. The light distribution exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. There is no strong evidence of distinct spiral arms or prominent dust lanes. The color profile appears relatively uniform, with a subtle shift toward redder hues in the central region compared to the slightly bluer outskirts. This may indicate an older stellar population in the core and ongoing or more recent star formation at larger radii. The overall structure seems relatively undisturbed, showing no major signs of ongoing merging activity or significant tidal distortions. Faint, diffuse features are present, suggesting some possible minor interactions. Overall, the galaxy appears to be a fairly massive system at an intermediate redshift, exhibiting characteristics consistent with an early-type galaxy in a relatively quiescent state.
