The galaxy presents a centrally concentrated morphology, exhibiting a relatively smooth light distribution. The overall shape appears to be generally rounded, though subtle deviations suggest a slight ellipticity. There is a color gradient observed, with the central region displaying a yellowish-white hue, which may indicate an older stellar population. The outer regions show a bluer tint suggesting the presence of more recent star formation, although this is not prominent. The image does not provide clear visual evidence of spiral arms or a well-defined disk structure. The galaxy appears to be relatively undisturbed, without strong indications of ongoing major merger activity. There are some subtle signs of minor interaction, possibly minor disturbances.
