The galaxy appears as an elliptical or lenticular structure. It presents a smooth, relatively featureless profile, lacking prominent spiral arms or significant dust lanes. The light distribution is centrally concentrated with a gradual falloff in intensity towards the outer regions. The central region shows a yellowish hue, likely indicating an older stellar population. The outer regions exhibit a slightly bluer color, suggesting the presence of some younger stars, although not in a well-defined disk structure. The overall shape is elongated, with a cigar-like appearance. There is no visually obvious evidence of ongoing major merger activity, though some minor disturbance or tidal features cannot be entirely ruled out based on this image alone.
