The galaxy presents a generally smooth and rounded morphology. The light profile appears concentrated, with a bright, yellowish core indicative of an older stellar population and/or significant dust obscuration. There is little evidence of spiral arm structure or distinct features; the galaxy appears largely featureless in the available image resolution. The color gradient suggests a relatively uniform distribution of stellar populations throughout the galaxy's visible extent, with a possible slight bluing towards the outer regions. There are no clear signs of ongoing major mergers or tidal disturbances.
