The galaxy presents as a moderately bright, somewhat elliptical structure. The light distribution is relatively smooth, suggesting a lack of prominent spiral arms. A slight elongation is visible, implying a deviation from perfect circularity, potentially approaching a cigar shape. The core region exhibits a higher concentration of luminosity compared to the outer regions, with the light gradually fading away from the center. The color profile indicates a bias toward the redder end of the spectrum, particularly in the central bulge. There may be some minor distortions or irregularities present within the galaxy's overall shape, perhaps indicative of a past or ongoing interaction, though these features are not pronounced. Overall, the galaxy appears to be a relatively evolved system with a predominantly older stellar population.
