The galaxy presents as a relatively smooth, elongated structure. The light distribution appears centrally concentrated, with a noticeable bulge or core region. The overall form factor of the galaxy is cigar-shaped, with a length that significantly exceeds its width. There appears to be minimal evidence of prominent spiral arms or distinct disk features. The galaxy's light profile fades gradually toward its outer edges, suggesting a lack of sharp boundaries. The galaxy displays a moderate red color, indicative of an older stellar population. There is no indication of significant ongoing star formation. The absence of pronounced disturbances suggests that the galaxy has not undergone a major merger event recently. The structure appears relatively undisturbed, and the light profile is well-behaved.