The galaxy appears to be a relatively smooth, elliptical-like object, exhibiting a concentrated central bulge. The light distribution suggests a spheroidal morphology, with a gradual decrease in luminosity from the core outwards. There is no discernible spiral arm structure or prominent disk component visible. The galaxy presents a yellowish hue, which suggests a stellar population dominated by older, redder stars. Some slight blue tinges appear in the outskirts of the galaxy which may indicate recent star formation. The galaxy's overall form is only slightly elongated. There is no evidence of tidal tails, strong gravitational lensing effects, or significant dust lanes. The galaxy does not obviously interact with other nearby galaxies.
