The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, featureless morphology. Its shape is elongated, roughly cigar-shaped, suggesting a departure from perfect circularity. There is no discernible spiral arm structure or distinct dust lanes. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The primary color is a greenish-blue hue, possibly indicating a population of relatively young, hot stars within the galaxy, or perhaps the effects of redshift. No obvious signs of major mergers or significant tidal disturbances are visible, though subtle asymmetries may indicate minor interactions or past accretion events.
