The galaxy presents a generally smooth morphology, suggesting a lack of significant spiral arm structure or prominent dust lanes. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. The galaxy exhibits a slightly elongated shape, deviating from a perfect circular form. The color profile is relatively uniform across the galaxy, with a yellowish-red hue indicative of an older stellar population and a potentially low star formation rate. There is no clear evidence of ongoing major merger activity, although some minor disturbances or tidal features cannot be entirely ruled out based on this image alone.
