The galaxy presents an overall elliptical morphology, with a relatively smooth, diffuse appearance. The central region exhibits a higher surface brightness and a yellowish hue, likely indicative of an older stellar population. Moving outward from the core, the light becomes bluer and fainter, suggesting the presence of some younger stars or a more dispersed stellar distribution in the outer regions. The galaxy appears to be mostly unperturbed, showing no obvious signs of major mergers or tidal interactions. The overall shape is somewhat elongated, with a cigar-like appearance. There is a faint irregularity on one side of the galaxy which could suggest a minor disturbance.
