The galaxy presents as a relatively smooth and centrally concentrated object. Its overall shape appears elliptical or lenticular, with a noticeable elongation. The central region exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outwards from the center, the color transitions to a slightly redder shade, which suggests the presence of a mix of intermediate-age and older stars in the outer regions. Faint blue patches may be present, albeit subdued, suggesting a low level of ongoing star formation. There are no prominent spiral arms or significant dust lanes visible. There is no obvious evidence of a major ongoing merger, although there appears to be a minor asymmetry or disturbance in its morphology, suggesting that the galaxy might have undergone a minor interaction or merger event in the past. 
