The galaxy presents as an elliptical or lenticular type, appearing elongated with a cigar-like shape. Its central region exhibits a concentrated and bright intensity, suggesting a substantial bulge component. Progressing outwards from the center, the luminosity gradually decreases. The galaxy displays a reddish hue throughout its structure, implying a population of older stars and/or significant dust obscuration. There is a subtle hint of what may be a disk component with very faint spiral structure, but further data is required to confirm this. Overall, the galaxy appears relatively isolated, showing no obvious signs of tidal interactions or ongoing mergers. The surrounding area is devoid of significant star formation regions, reinforcing the characterization of an older stellar population.
