The object appears to be an elliptical galaxy, exhibiting a generally smooth morphology with no readily discernible spiral arms or disk-like structures. The galaxy presents an elongated shape, leaning towards a cigar-like appearance rather than being perfectly spherical. The light distribution appears concentrated towards the center, indicating a central bulge. There is little evidence of ongoing major merger activity or significant tidal disturbances. The galaxy appears to be a relatively isolated system. The color suggests an older stellar population.
