The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is a slight elongation, with an aspect ratio tending towards round rather than cigar-shaped. The central region exhibits a yellowish-white hue, suggesting an older stellar population. Fainter, diffuse light extends outwards from the center, showing a faint blue tint. The surrounding outer regions display subtle variations in color and intensity, indicating some heterogeneity in stellar populations. No distinct spiral arms or prominent dust lanes are discernible. There appears to be no major or minor disturbances in the galaxy's structure, and it is not currently undergoing a major merger. 
