This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless morphology. It has a somewhat elongated, cigar-shaped form. The color distribution shows a concentration of bluer light towards the central region, potentially indicating a population of younger stars or ongoing star formation within the core, however, this appears to be minimal. The outer regions display a redder hue, suggesting an older stellar population. There is no apparent spiral structure, distinct dust lanes, or signs of active galactic nuclei. The overall structure seems largely undisturbed, lacking evidence of any recent major mergers or significant tidal interactions. It appears to be a relatively isolated system, evolving passively.
