The galaxy presents as a moderately luminous, elongated structure. Its color profile indicates a generally redder population of stars, suggesting an older stellar population and relatively low current star formation. The central bulge appears prominent, with a smooth and diffuse light distribution. The galaxy exhibits a cigar-like morphology, indicating that we are likely viewing it at a significant inclination. There is a lack of any apparent spiral arm structure or significant dust lanes. The overall appearance is consistent with an elliptical galaxy, or potentially a highly inclined lenticular galaxy.
