The galaxy appears to be an elongated, elliptical structure, exhibiting a smooth morphology with a bright, concentrated central bulge. The galaxy's light profile suggests a relatively old stellar population, concentrated in the core with a gradual fading towards the outer regions. There is a faint blue region towards the lower portion of the disk, suggesting some star formation. The overall shape is highly elongated, appearing almost cigar-shaped. The galaxy does not present any obvious signs of strong tidal disturbances or major mergers. A possible companion galaxy is close by, so there may be some type of interaction.
