The galaxy presents as a moderately luminous, elongated structure with a smooth overall appearance. Its shape is notably cigar-shaped, lacking a well-defined disk structure. The light distribution suggests a dominant central bulge, with a gradual decrease in surface brightness towards the outer regions. The color profile indicates a general red hue, with slight variations suggesting potential regions of ongoing star formation. No obvious signs of spiral arms or significant dust lanes are apparent. There are no indications of any ongoing major merging events or significant tidal disturbances.
