The observed galaxy presents a generally smooth, elongated morphology, approximating a cigar shape in appearance. The light distribution suggests a concentrated central bulge that transitions smoothly into a more diffuse, surrounding disk. There is a notable color gradient, with the central regions appearing more yellowish-white, potentially indicating an older stellar population. Progressing outward from the center, there is a subtle shift towards bluer hues in the outer regions, suggestive of more recent or ongoing star formation activity. Overall the galaxy exhibits no apparent strong distortions or tidal features, indicating a relatively quiescent state.
