The galaxy appears as an elongated, cigar-shaped structure. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars and possibly a central supermassive black hole. The color gradient transitions from a yellowish-white core to a more reddish hue in the outer regions. This color suggests the presence of an older stellar population and less active star formation in the galaxy's outer regions. There are no distinct spiral arm features visible. The galaxy appears relatively smooth, with only minor irregularities in its overall structure, not showing any significant merging or tidal disturbance features. The observed morphology suggests the galaxy may be an elliptical or lenticular type galaxy.
