The galaxy exhibits a largely smooth morphology, with a dominant central bulge. The shape is approximately round, although there is a slight elongation. The color profile indicates a reddish hue, suggesting an older stellar population and potentially a lower rate of star formation. There appears to be evidence of a possible interaction or merger, with some distortion visible in the galaxy's overall structure. This is further supported by the presence of what might be a tidal tail or bridge extending from the main body. The galaxy is relatively compact, with a noticeable concentration of light in its core.
