The galaxy presents as a lenticular or possibly an elliptical type. The central bulge exhibits a smooth, concentrated light distribution, appearing largely spheroidal and dominating the galaxy's overall luminosity. There is a lack of distinct spiral arm structure or significant dust lane features, which contribute to this smoothness, and cigar-like shape. The color profile is relatively uniform across the galaxy, trending towards redder hues, particularly in the central bulge, suggesting an older stellar population. The galaxy has a moderate redshift value, placing it at a considerable cosmological distance. Any disk, if present, is viewed edge-on. There is some indication of minor tidal disturbance or interactions, evidenced by slight asymmetries in the outer regions, or potential faint streams, but these are not prominent. Star formation rate is relatively low.
