The galaxy appears to be a spiral galaxy, possibly an intermediate spiral, exhibiting a notable central bulge that transitions into a less defined disk. The bulge has a yellowish-orange hue, potentially indicating an older stellar population. The disk presents a mottled texture with subtle indications of spiral arm structure.

There is a slight irregularity to the galaxy's morphology, particularly at the lower edge, with a reddish region that could suggest either active star formation or the influence of tidal interactions, however this could also simply be noise or a foreground/background object. Overall, the galaxy seems to be relatively undisturbed, but close inspection shows it may be undergoing some sort of interaction.
