The galaxy presents an overall smooth morphology, appearing largely featureless upon initial inspection. The light profile is centrally concentrated, exhibiting a gradual falloff in surface brightness from the core outwards. The galaxy's shape is significantly elongated, displaying a cigar-like appearance. There are no apparent signs of tidal tails, strong asymmetries, or multiple nuclei, suggesting it is not currently undergoing a major merger, however, a minor disturbance is possible. The color profile suggests an older stellar population, the yellow to red hues of the galaxy are more dominant compared to blue hues associated with star formation. The galaxy's relatively high luminosity indicates a substantial stellar mass.
