The galaxy presents as a somewhat elongated structure. The light distribution is mostly concentrated in the central region, with a visible extension or arm-like feature emanating from one side. There appears to be a noticeable color gradient across the galaxy; the core region exhibits a yellowish-orange hue, possibly indicating an older stellar population, whereas the outer extension shows a bluer tint, suggesting the presence of younger, hotter stars or ongoing star formation. There are potential signs of minor disruption in the galactic structure. The galaxy’s overall morphology does not clearly fit into a distinct category, such as elliptical or spiral, it looks like an intermediate between the two.
