The galaxy presents a generally smooth morphology, suggesting a classification towards the elliptical end of the Hubble sequence. The light distribution is concentrated towards the center, with a notable central bulge exhibiting a yellowish hue. The outer regions of the galaxy are less defined, gradually fading into the background sky. There is a slight elongation to the overall shape, deviating marginally from a perfectly circular form. No distinct spiral arms or prominent dust lanes are apparent, lending further credence to the classification as an elliptical galaxy. There is a lack of significant signs of recent or ongoing major mergers.
