The galaxy presents as a smooth, elongated structure. It exhibits a centrally concentrated bulge, appearing bright and yellowish in color, which diminishes in intensity towards the outer regions. The galaxy displays an overall cigar-like shape with no apparent spiral arm structure or prominent dust lanes visible in this image. The light distribution suggests a relatively homogenous stellar population within the bulge. There is no evidence of active galactic nuclei or any significant ongoing merging activity. The outer regions of the galaxy appear somewhat diffuse, gradually fading into the background. Based on the observed characteristics, this galaxy is potentially an elliptical or lenticular type galaxy.
