The galaxy presents an elongated, cigar-like morphology, suggesting an elliptical or lenticular classification, viewed at a significant angle. The light distribution is relatively smooth, with a concentrated central bulge and a diffuse halo. A slight color gradient can be observed, trending towards redder hues in the central region and subtly bluer tones in the outer regions. No distinct spiral arms or prominent dust lanes are apparent. There is no obvious presence of tidal tails or other signs of recent major mergers. The galaxy appears to be relatively isolated, with no immediate, gravitationally interacting companions visible in the field.
