The galaxy appears as a centrally concentrated, smooth object with a slightly elongated morphology. The light profile suggests a gradual decline in brightness from the center outwards. The core region exhibits a brighter, more intense glow, transitioning into a fainter halo. There is no apparent spiral structure, bar, or significant dust lane visible in this image. The object's overall shape is more akin to a cigar. There is no obvious sign of any major ongoing merger activity or tidal disturbances. The galaxy's color profile indicates it is likely composed of aging stellar populations and exhibiting a low rate of current star formation activity.
