The galaxy presents as a relatively smooth, elliptical-like structure, elongated with a cigar-shaped morphology. Its core exhibits a bright, concentrated luminosity, shifting towards redder wavelengths. The outer regions display a gradual decline in surface brightness, with some bluer, green emissions. There is little evidence of spiral arm structure, though some disk-like features may be present. The galaxy does not appear to be undergoing any major merging events or significant disturbances based on the overall symmetry of the light distribution. The galaxy appears to be a quiescent system, with a population of aging stars contributing to its reddish hue, though some star formation might be present in the bluer, green regions.
