The galaxy presents as a small, elongated structure, approximately cigar-shaped in appearance. Its color profile appears relatively uniform, with a slight reddish hue overall. There is little evidence of distinct spiral arms or a prominent central bulge. The light distribution appears smooth, lacking significant clumpy or irregular features, indicating a relatively homogenous stellar population or a significant amount of dust obscuring finer details. There are no apparent signs of ongoing major mergers or tidal disturbances. Based on these observations, the galaxy appears to be a relatively quiescent system. Further spectral data would be beneficial to analyze its star formation rate and stellar population in detail.
