The galaxy presents as a relatively smooth object with a slightly elongated, cigar-shaped morphology. The light distribution appears to be centrally concentrated, exhibiting a radial gradient in surface brightness decreasing from the core outward. There's a subtle hint of asymmetry in the isophotes, perhaps indicative of a minor tidal interaction or internal disturbance but not enough to suggest a merger. The color profile is moderately uniform across the galaxy, with a subtle reddish-yellow hue, suggesting an older stellar population with a lower rate of star formation. No distinct spiral arms or prominent dust lanes are discernible in the image. Overall, the galaxy appears to be a mature system with a smooth light distribution, lacking strong features indicative of ongoing active star formation or major disturbances.
