The galaxy presents a generally smooth morphology. It has a distinct, concentrated bulge region that exhibits a reddish hue, potentially indicating an older stellar population. Surrounding the bulge is a less concentrated, somewhat flattened disk component. This disk displays a bluer color, suggestive of more recent or ongoing star formation. There may be very faint, subtle indications of spiral arm structure within the disk, but the overall appearance is predominantly smooth. The galaxy's shape appears nearly round, with minimal elongation. There is no obvious evidence of any major tidal disturbances or ongoing merger activity; the system appears to be relatively isolated and relaxed.
