The galaxy presents as an elongated, cigar-shaped structure with a primarily smooth morphology. The central region exhibits a concentrated luminosity, appearing more luminous than the outer regions. The color profile indicates a generally redder hue, potentially indicative of an older stellar population. There is little evidence of spiral arm structure or significant dust lanes. Faint, diffuse extensions can be tentatively identified at the top and bottom of the galaxy, with hints of blue, although their precise nature and connection to the main galactic body requires further investigation. The overall impression is that of an early-type galaxy at a moderate redshift. There is a slight disturbance in the upper region of the galaxy.
