The galaxy presents as a relatively smooth, featureless object, potentially an elliptical or lenticular type. Its overall shape is elongated, exhibiting a cigar-like morphology. There is a central concentration of light that decreases gradually towards the edges, indicating a bulge-dominated structure. The galaxy displays a blue hue, suggesting the presence of some young stars and active star formation, however, this does not appear to be very significant. No distinct spiral arms or prominent dust lanes are visible. There is no obvious signs of any interactions or ongoing mergers with other galaxies. The overall color suggests a population of moderately old stars.
