The galaxy presents a somewhat elongated morphology, appearing cigar-shaped along its major axis. The luminosity profile suggests a central bulge, with a gradual decrease in surface brightness moving outwards. The color distribution indicates a possible redder core region, perhaps indicative of an older stellar population. There may be a slight warping or tidal disturbance at one end of the galaxy, with a hint of a faint extended structure. Overall, the galaxy exhibits features that could possibly be interpreted as a spiral galaxy seen edge-on, or an elliptical galaxy with some minor disturbance. Further spectral analysis would be needed to confirm these morphological assessments.
