The galaxy presents as an elongated, cigar-shaped object, suggesting it is likely an elliptical galaxy viewed edge-on, or a highly inclined spiral galaxy. The light distribution is relatively smooth and concentrated towards the center. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. Fainter blue-ish regions are visible extending from the galaxy's center, implying the possibility of recent or ongoing star formation within these regions. There is no obvious spiral arm structure. There is no evidence of a major merger or significant tidal disturbances.