The galaxy appears to be an elliptical galaxy, characterized by its smooth, concentrated light profile. Its overall shape is approximately spheroidal, though slightly elongated. The central region exhibits a bright, yellowish hue, possibly indicating a population of older, redder stars. Progressing outwards from the center, the galaxy becomes dimmer, with a subtle decrease in the concentration of light. There are indications of faint, blueish-green surrounding the core, though they are not a spiral feature; they may signify some star forming regions within the galaxy, albeit at a low rate. The galaxy does not show evidence of any major disturbances or recent merger activity based on a simple visual inspection.
