The galaxy presents as an elongated, spindle-shaped object, indicative of an elliptical morphology viewed at an oblique angle. The central region exhibits a concentrated, bright core, suggesting a high density of stars. The color profile is dominated by yellowish-white hues in the central regions, transitioning to a redder tint towards the outer edges, which could imply a gradient in stellar populations and/or dust content. There's little evidence of distinct spiral arms or prominent dust lanes from this viewing angle. Overall, the galaxy appears to be relatively smooth and featureless, save for the color variation indicating some level of spatial diversity. There is no obvious evidence of any ongoing major merger activity. A minor disturbance cannot be ruled out. The elongated shape suggests a possible cigar-like form factor.
