The galaxy appears as an elongated, somewhat cigar-shaped structure. Its light profile suggests a relatively smooth distribution, with a bright, concentrated central bulge region that fades gradually towards the outer edges. There is evidence of a disk component, although it is not distinctly spiral. Instead, the disk appears more lenticular in nature, showing a diffuse, flattened structure extending beyond the central bulge. The galaxy exhibits a reddish hue, indicating a potentially older stellar population with lower rates of ongoing star formation. There are no signs of significant tidal disturbances or major mergers in the immediate vicinity, although subtle asymmetries in the outer regions cannot be entirely ruled out.
