The galaxy presents as a central bulge with a flattened disk-like structure. The central bulge exhibits a smooth, relatively uniform light distribution, suggesting an older stellar population dominating this region. The disk component displays a less structured appearance with a hint of spiral arms, though these are not clearly defined, possibly obscured by dust or viewed at a shallow angle. The colors indicate a range of stellar populations. The central regions appear more yellow-red, indicative of older stars, while the outer disk shows bluer hues, suggesting the presence of younger, hotter stars and ongoing star formation, particularly on one side. There appears to be a minor disturbance or a possible merger event with a smaller galaxy, as evidenced by a slight asymmetry and a possible tidal tail or stream of stars extending from one side of the disk. Overall, the galaxy presents an intermediate morphology, potentially a late-type spiral galaxy undergoing some interaction.
