The galaxy presents a generally smooth morphology, with a notable central bulge that appears somewhat spherical in shape. The main body exhibits a diffuse, elliptical profile, showing a transition from a brighter, more concentrated core to a fainter outer region. While the overall structure is predominantly smooth, there are subtle indications of possible minor disturbances or interactions, as evidenced by slight irregularities in its extended halo. The color distribution suggests the presence of a mix of stellar populations. The central bulge displays a warmer, yellowish hue, which could indicate the presence of older, redder stars. In contrast, the outer regions have a more subtle blueish tinge, which may indicate some level of recent star formation activity, however minimal. No spiral arm structure is obviously visible.
