The galaxy presents as a smooth, elongated structure, strongly suggestive of an elliptical morphology. The central region exhibits a concentrated luminosity. Progressing outwards from the core, the light diffuses, indicating a lack of distinct spiral arms or prominent features. The color profile displays a generally red hue with a lack of blue areas, particularly near the center. This color profile suggests a stellar population dominated by older stars and/or a significant dust content obscuring bluer, younger stars. There are no strong indications of active star formation. The overall form is cigar-shaped, with no visible signs of significant tidal disturbances or ongoing merger events.
